[Ips-dsgr] IPS Daily Report - 13 December 03
rwc
rwc at ips.gov.au
Sun Dec 14 09:17:13 EST 2003
SUBJ: IPS DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 13/2330Z DECEMBER 2003 BY IPS RADIO AND SPACE SERVICES
FROM THE AUSTRALIAN SPACE FORECAST CENTRE
SUMMARY FOR 13 DECEMBER AND FORECAST FOR 14 DECEMBER - 16 DECEMBER
STATUS INDICATORS SOL:GREEN MAG:** YELLOW ** ION: **YELLOW**
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1A. SOLAR SUMMARY
Activity 13 Dec: Very low
Flares: none.
Observed 10.7 cm flux/Equivalent Sunspot Number for 13 Dec: 88/32
1B. SOLAR FORECAST
14 Dec 15 Dec 16 Dec
Activity Low Low Low
Fadeouts None expected None expected None expected
10.7cm/SSN 95/41 100/48 100/48
COMMENT: The sun has remained flare quiet over the past 24 hours.
Solar wind remains elevated at around 700km/sec with the north-south
comonent of the interplanetary magnetic field remaining mildly
southward over the UT day. Recurrence suggests that solar wind
speed should ease over coming days. Elecated solar wind speed
due to coronal hole high speed wind stream.
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2A. MAGNETIC SUMMARY
Geomagnetic field for Australian Region 13 Dec: Quiet to Active
Estimated Indices 13 Dec : A K
Australian Region 16 3333 4333
Darwin 13 2223 4333
Townsville 20 2333 5433
Learmonth 21 3334 5333
Culgoora 16 3333 4333
Canberra 16 3333 4333
Hobart 21 3444 4333
Casey(Ant) 21 ---4 4333
Observed Regional daily pc3 Indices 13 DEC :
Townsville 17 (Quiet)
Learmonth 69 (Active)
Culgoora 99 (Minor storm)
Canberra 158 (Severe storm)
Hobart 113 (Major storm)
Pc3 pulsations are high frequency (10-45 second period) variations
of the Earths magnetic field. Daily pc3 indices are the daily sum
of 20 minute pc3 indices for that station.
Estimated AFr/Ap Indices 13 Dec : A
Fredericksburg 25
Planetary 27
Observed AFr/Ap Indices 12 Dec : A K
Fredericksburg 17
Planetary 23 4443 4345
2B. MAGNETIC FORECAST
Date Ap Conditions
14 Dec 20 active
15 Dec 14 Unsettled to Active
16 Dec 10 Quiet to Unsettled
COMMENT: Active conditions probable next two days, with a gradual
decline in activity levels on day three, as the Earth is expected
to leave the solar coronal hole high speed wind stream.
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3A. GLOBAL HF PROPAGATION SUMMARY
Latitude Band
Date Low Middle High
13 Dec Normal Fair-normal Poor-fair
PCA Event : No event.
3B. GLOBAL HF PROPAGATION FORECAST
Latitude Band
Date Low Middle High
14 Dec Normal Normal-Fair Fair
15 Dec Normal Normal Normal-Fair
16 Dec Normal Normal Normal-Fair
COMMENT: General trend of improving HF conditions are likely at
mid to high latitudes over the next day few days as the Earth
leaves the coronal hole high speed wind stream.
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4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY
Date T index
13 Dec 53
Observed Australian Regional MUFs
Equatorial PNG Region:
Near predicted monthly values during local day,
Enhanced by 45% during local night.
Northern Australian Region:
Near predicted monthly values during local day,
Enhanced by 20% during local night.
Southern Australian and New Zealand Region:
Depressed by 15% during local day,
Near predicted monthly values during local night.
Antarctic Region (Casey/Scott Base):
Near predicted monthly values early in the UT day.
Depressed 15% later in UT day. Blanketing sporadic
E observed.
Predicted Monthly T index for December: 50
4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date T index MUFs
14 Dec 45 depressed 10 to 15%/near predicted monthly values
15 Dec 50 depressed 10 to 15%/near predicted monthly values
16 Dec 55 Near predicted monthly values
COMMENT: Mild depressions possible after local dawn for southern
Aus/NZ region. MUFs are expected to generally return to near
predicted monthly values over coming days, as the Earth leaves
the coronal hole high speed wind stream.
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5. SPACE ENVIRONMENT SUMMARY
GOES satellite data for 12 Dec
Daily Proton Fluence >1 MeV: 5.1E+06
Daily Proton Fluence >10 MeV: 1.2E+04
Daily Electron Fluence >2 MeV: 6.30E+08 (high)
X-ray background: A7.4
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
ACE Satellite Solar Wind Day Averaged Data for 12 Dec
Speed: 755 km/sec Density: 1.1 p/cc Temp: 275000 K Bz: -2 nT
(Courtesy Space Environment Center, Boulder USA)
ACE data can be incorrect during strong proton events.
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